July 24, 2009 : Workshop on the Mid-infrared Instrument for TAO 6.5m telescope
A workshop on the mid-infrared instrument for TAO 6.5m telescope (TAOMIR) was held
on July 24, 2009. Sufficient exchanges of opinions about the specifications, the
performances, and the scientific cases of the TAOMIR were conducted. We continue to
develop the TAOMIR in order to be a widely used instrument for many astronomers.
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▲ TAOMIR workshop
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Date: | 2009/07/24(Fri) 11:00 - 18:00 |
Venue: | Lecture room at the Institute of Astronomy, UT |
Program: | 11:00-11:05 | Remarks | Miyata |
Details of the instruments |
11:05-11:20 | MAX38: a prototype camera of the TAOMIR | Nakamura, Asano |
11:20-11:50 | TAOMIR | Miyata |
11:50-12:45 | Lunch |
Stars |
12:45-13:00 | Imaging/Spectroscopic Monitoring of nearby variable stars in MIR | Ita |
13:00-13:15 | Mira variables in the galactic center seen by TAO | Matsunaga |
13:15-13:30 | Investigations of MOLsphere | Tanabe |
Star and Planet formation |
13:30-13:45 | Observations of dust around young stars | Fujiwara |
13:45-14:00 | Monitoring observations of disks, and some comments on the instrument spec. | Kataza |
14:00-14:15 | Massive star formation | Okamoto |
14:15-14:30 | Break |
Interstellar Medium |
14:30-14:45 | Science cases of MIR polarimetry | Honda |
14:45-15:00 | Interstellar medium studied with TAOMIR | Sakon |
Solar system |
15:00-15:15 | Small bodies in the solar system studied with TAOMIR | Otsubo |
15:15-15:30 | MIR imaging observations of comets | Ishiguro |
15:30-15:45 | Planetary magnetosphere observed in MIR | Yoneda |
Synergy with Radio obsevations |
15:45-16:00 | Synergy of TAOMIR and ALMA/ASTE | Kohno |
16:00-16:15 | Break |
Extragalaxy |
16:15-16:30 | Mass estimation of CDM subhalo with MIR monitoring observationsMinezaki | Minezaki |
16:30-16:45 | Follow-ups of MIR all sky survey: Searching for dust obscured AGNs | Oyabu |
16:45-17:00 | Break |
TAOMIR Science WG |
17:00-17:15 | Summary and TAOMIR science WG | Sako |
Discussion |
17:15-18:00 | Discussion | Miyata |
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